The frequency of circumstellar envelopes among TMSS stars

Details The frequency of circumstellar envelopes among TMSS stars The frequency of circumstellar envelopes among TMSS stars

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..149b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 149-150

Astronomy and Astrophysics

Astronomy

Sky Surveys (Astronomy), Star Distribution, Stars, Stellar Color, Stellar Envelopes, Stellar Spectra, Graphs (Charts), Oxygen, Ratios, Red Shift, Stellar Spectrophotometry

Scientific paper

We investigated the distribution of Neugebauer and Leighton's two micron
survey (TMSS) stars on the (K - (12);(12) - (25)) and ((12) - (25);(25)
- 60)) planes. The frequency of circumstellar emission objects among B-K
type stars is less than 5% while it reaches about 20% at M, 80% at stars
with unknown spectra and 90% at carbon stars.

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